Three-dimensional modeling of ionized gas - II. Spectral energy distributions of massive and very massive stars in stationary and time-dependent modeling of the ionization of metals in H ii regions

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Volume 583 (November 2015)

A&A, 583 (2015) A63

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Table 4

Numerical values of the integrals of ionizing photons emitted per second for the ionization stages of H, He, He⁺, O⁺, Ne⁺, and S⁺, as well as the luminosity at the reference wavelength λ = 5480 ^˚A.

Model	Z/Z_⊙	log Q_H	log Q_He	log Q_He⁺	log Q_O⁺	log Q_Ne⁺	log Q_S⁺	L_ν(5480 ^˚A)
								(10²² erg/s/Hz)

Dwarfs

D-30	0.1	47.60	45.02	38.97	42.92	41.10	45.95	3.85
	0.4	47.58	45.03	36.49	42.89	41.12	45.82	4.09
	1.0	47.56	45.09	35.23	42.96	41.31	45.76	4.17
	2.0	47.71	45.34	35.62	43.26	41.62	45.86	4.06
D-35	0.1	48.67	47.58	42.15	46.55	45.50	47.74	4.22
	0.4	48.66	47.56	41.51	46.29	44.53	47.71	4.21
	1.0	48.68	47.58	37.41	46.17	44.22	47.70	4.36
	2.0	48.68	47.49	37.61	45.83	44.00	47.63	4.45
D-40	0.1	49.09	48.43	43.95	47.76	46.97	48.51	4.19
	0.4	49.08	48.35	43.67	47.47	46.41	48.44	4.30
	1.0	49.08	48.31	43.78	47.30	46.17	48.41	4.38
	2.0	49.06	48.25	43.87	47.07	45.98	48.36	4.53
D-45	0.1	49.53	48.96	45.22	48.37	47.70	49.02	6.60
	0.4	49.52	48.89	45.24	48.19	47.43	48.97	7.27
	1.0	49.50	48.83	45.12	47.97	47.12	48.92	7.43
	2.0	49.50	48.78	45.00	47.77	46.84	48.88	7.75
D-50	0.1	49.76	49.26	46.07	48.72	48.11	49.32	7.69
	0.4	49.75	49.22	46.17	48.60	47.91	49.29	8.44
	1.0	49.74	49.19	46.04	48.42	47.64	49.26	8.79
	2.0	49.74	49.16	45.77	48.28	47.41	49.23	9.50
D-55	0.1	50.14	49.71	46.88	49.23	48.70	49.76	12.93
	0.4	50.14	49.72	47.18	49.19	48.54	49.77	13.62
	1.0	50.14	49.72	47.11	49.11	48.36	49.77	14.07
	2.0	50.14	49.69	46.76	48.90	48.11	49.74	16.04

Supergiants

S-30	0.1	49.27	48.00	37.72	46.55	44.90	48.16	22.22
	0.4	49.25	47.88	36.04	46.26	44.06	48.04	22.97
	1.0	49.25	47.85	35.32	45.54	43.35	48.01	22.98
	2.0	49.22	47.78	35.29	45.18	41.85	47.94	23.90
S-35	0.1	49.48	48.63	37.34	47.73	46.82	48.73	15.54
	0.4	49.47	48.55	37.45	47.25	46.18	48.66	16.27
	1.0	49.47	48.47	37.50	46.83	45.92	48.59	16.28
	2.0	49.47	48.36	36.56	46.21	45.55	48.49	16.98
S-40	0.1	49.67	49.01	45.06	48.32	47.51	49.10	15.01
	0.4	49.67	48.93	38.94	48.03	47.11	49.03	15.70
	1.0	49.66	48.81	38.54	47.57	46.70	48.95	16.68
	2.0	49.66	48.70	38.06	47.07	46.27	48.86	18.15
S-45	0.1	49.98	49.41	45.97	48.81	48.12	49.47	19.12
	0.4	49.97	49.35	45.79	48.67	47.78	49.43	19.62
	1.0	49.97	49.28	39.23	48.30	47.37	49.36	22.52
	2.0	49.98	49.19	38.85	47.92	46.97	49.29	23.92
S-50	0.1	50.21	49.73	46.76	49.21	48.59	49.78	20.66
	0.4	50.20	49.70	46.79	49.08	48.34	49.76	21.97
	1.0	50.20	49.69	46.41	48.88	48.06	49.75	23.66
	2.0	50.21	49.69	46.23	48.84	47.81	49.75	24.80

Notes. With respect to their ionization energies these ions are important in the context of emission line diagnostics. The integrals are defined as , where hν_X is the ionization energy of ion X. (The ionization energy is 1.72 Ryd for S ii, 1.81 Ryd for He i, 2.77 Ryd for O ii, and 3.01 Ryd for Ne ii.)

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